DTIC ADA164458: Peak-Flux-Density Spectra of Large Solar Radio Bursts and Proton Emission from Flares.
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DTIC ADA164458: Peak-Flux-Density Spectra of Large Solar Radio Bursts and Proton Emission from Flares.
- Publication date
- 1985-08-19
- Topics
- DTIC Archive, Cliver,E W, AIR FORCE GEOPHYSICS LAB HANSCOM AFB MA, *SOLAR FLARES, *RADIOFREQUENCY SPECTROSCOPY, *RADIO SOURCES(ASTRONOMY), FREQUENCY, EMISSION, PEAK VALUES, ACCELERATION, SHOCK WAVES, MICROWAVES, PROTONS, ELECTRONS, SPECTRA, MEASURING INSTRUMENTS, RADIO SIGNALS, SOLAR CORONA, FLASHES, BURST TRANSMISSION, SOLAR DISTURBANCES,
- Collection
- dticarchive; additional_collections
- Language
- English
We have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar proton events for approx 200 large (Sp( or = 2GHz) or = 800 solar flux uits (sfu) microwave burst (1965 - 1979). The radio spectra fell into two basic classes: (a) U-shaped with two maxima ( or = 800 sfu) in the range from 200 MHz to or = 10 GHz (59 percent of all events), and (b) cutoff spectra with a maximum or = 800 sfu at f or = 2 GHz and Sp (200 MHz) 100 sfu (18 percent). Nine percent of the events had intermediate spectra with a maximum or = 800 sfu at f or = 2 GHz and 100 sfu or = Sp (200 MHz) 800 sfu. We were unable to classify 15 percent of the events because of incomplete data. The associations of the three classes of spectra with Type II (and/or Type IV) meter wavelenght bursts and 10 MeV proton events of any size ( or = 0.01 pr per sq cm per sec per sr) are as follows: U-shaped Type II/IV (90 percent of large microwave bursts with U-shaped spectra are associated with Type II/IV events), protons (77 percent); intermediate Type II/IV (78 percent), protons (73 percent); and cutoff Type II/IV (22 percent), protons (33 percent). These statistics affirm various lines of evidence linking coronal shock waves and interplanetary proton events. They also suggest that the meter wavelength branch of the U-shaped spectrum may be attributable to second phase (vs flash phase) accelerated electrons.
- Addeddate
- 2018-02-05 19:51:06
- Foldoutcount
- 0
- Identifier
- DTIC_ADA164458
- Identifier-ark
- ark:/13960/t79s8799r
- Ocr_converted
- abbyy-to-hocr 1.1.37
- Ocr_module_version
- 0.0.21
- Page_number_confidence
- 43
- Page_number_module_version
- 1.0.3
- Pages
- 65
- Ppi
- 300
- Year
- 1985
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